Surface magnetic fields on two accreting T Tauri stars: CV Cha and CR Cha

Monthly Notices of the Royal Astronomical Society

Volumn 398, Issue 1, 2009, Pages 189-200

  Hussain, G A J ^a   Collier Cameron, A ^b   Jardine, M M ^b   Dunstone, N ^b   Velez, J Ramirez ^c   Stempels, H C ^b   Donati, J F ^d   Semel, M ^c   Aulanier, G ^c   Harries, T ^e   Bouvier, J ^f   Dougados, C ^f   Ferreira, J ^f   Carter, B D ^g   Lawson, W A ^h  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c OBSERVATOIRE DE PARIS   (France)

^d OBSERVATOIRE MIDI PYRÉNÉES   (France)

^e UNIVERSITY OF EXETER   (United Kingdom)

^f UNIV GRENOBLE ALPES   (France)

^g UNIVERSITY OF SOUTHERN QUEENSLAND   (Australia)

^h UNIVERSITY OF NEW SOUTH WALES   (Australia)

Author keywords

Open clusters and associations: Individual: Chamaeleon I; Stars: Formation; Stars: Imaging; Stars: Individual: CR Cha; Stars: Individual: CV Cha; Stars: Magnetic fields

Indexed keywords

LUMINANCE; STARS;

OPEN CLUSTER AND ASSOCIATION: INDIVIDUAL: CHAMELEON I; OPEN CLUSTERS AND ASSOCIATION: INDIVIDUAL; STAR: INDIVIDUAL: CR CHA; STAR: INDIVIDUAL: CV CHA; STARS FORMATION; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MAGNETIC FIELD; STARS:IMAGING; T TAURI STARS;

MAGNETIC FIELDS;

EID: 69449090456     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14881.x     Document Type: Article

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